Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ ZENODOarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Software . 2025
Data sources: ZENODO
ZENODO
Software . 2025
Data sources: Datacite
ZENODO
Software . 2025
Data sources: Datacite
versions View all 2 versions
addClaim

sblunt/eccentricities: Initial release

Authors: Blunt, Sarah;

sblunt/eccentricities: Initial release

Abstract

Welcome to the collection of code I wrote to perform the analysis in Blunt et al (2026): Evidence for a Peak at ~0.3 in the Eccentricity Distribution of Typical Super-Jovian Exoplanets (arXiv:2601.18877). Please feel free to raise an issue if you spot a bug or have a question. Here's a quick map for those looking to recreate the analysis: I'm starting from the assumption that you have access to the California Legacy individual fit posteriors (if you don't, reach out to BJ Fulton and he can share with you). Once you have the posteriors (I put them in a directory called lee_posteriors/run_final), run get_posteriors.py. This script grabs eccentricity, msini, and semimajor axis posteriors from lee_posteriors/run_final for the sample in my paper, uses importance resampling to obtain samples the posteriors assuming they were sampled under unifom priors on log(sma) and log(msini), and writes them as csvs to be injested into the HBM model. Next, run make_completeness_model.py, which computes a completeness model using publicly available injection-recovery tests (https://github.com/leerosenthalj/CLSI/tree/master/completeness/recoveries_all) Finally, you can run some hierarchical Bayesian models (HBM). run_histogram_full_marginalization.py uses the "accepted" model, which performs a full marginalization over inclination (see appendix A of paper). run_histogram.py performs a "cheat-y" marginalization-- instead of doing all the marginalization math, it assumes each msini posterior can be translated to a mass posterior by multiplying by random values of inclination drawn from a uniform distribution in cosi. This script can also be adapted to perform the fit in bins of msini, not mass, by simply setting each value drawn from cosi to be inc=90, rather than the random values. run_gaussian.py uses the same "cheat-y" marginalization as run_histogram.py, but the HBM model fit is a Gaussian, rather than a histogram. There are several plotting scripts in the plotting_scripts directory that will display the results. NOTE: I changed around some of the directories right before pushing and didn't recheck that everything works in the new organization. Forgive me, I busy. Please feel free to raise an issue if there's a bug you can't figure out. NOTE: There's some repeated code in run_gaussian.py, run_histogram_full_marginalziation.py, and run_histogram.py. Forgive me software engineering gods (and future me who will inevitably run into bugs for this reason).

Related Organizations
  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average